Computer Science – Numerical Analysis
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77...13d&link_type=abstract
Solar Physics, vol. 77, Apr. 1982, p. 13-26.
Computer Science
Numerical Analysis
11
Circular Polarization, Magnetic Flux, Photosphere, Solar Atmosphere, Solar Magnetic Field, Thermodynamic Properties, Atmospheric Models, Magnetic Field Configurations, Numerical Analysis, Sunspots
Scientific paper
The thermodynamic properties of magnetic flux tubes (MFTs) are investigated by means of a diagnostic method based on the observation of circular polarization signals in line pairs. Two lines of the same element are considered that have the same effective Lande factor and intensity profile in the mean photosphere. Any observed difference in the circular polarization signals of the lines is ascribed to thermodynamic structure of the MFT resulting in a differential weakening of the lines. The concept of response function for the ratio of circular polarization signals in two lines is introduced and its main properties are analyzed. Some detailed calculations for suitably selected line pairs are presented.
Landi Degl'Innocenti Egidio
Landolfi Marco
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